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researcher

J. Han

16 papers hereh-index 222k citations120 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author4
  • middle author4
  • last author6

Across the 15 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph15
  • astro-ph.SR1
same name
  • J. Han — 38 papers
  • J. Han — 23 papers, h 30
  • J. Han — 15 papers
  • J. Han — 12 papers, h 110
  • J. Han — 12 papers
  • J. Han — 10 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982009
most citedThe Galactic distribution of magnetic fields in molecular clouds and HII regions

50 citations · 165 across the 10 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006★ 50 cited

The Galactic distribution of magnetic fields in molecular clouds and HII regions

J. L. Han, J. S. Zhang

{Magnetic fields exist on all scales in our Galaxy. There is a controversy about whether the magnetic fields in molecular clouds are preserved from the permeated magnetic fields in…

astro-ph2006★ 33 cited

Spin-Kick Correlation in Neutron Stars: Alignment Conditions and Implications

Chen Wang, Dong Lai, JinLin Han

Recent observations of pulsar wind nebulae and radio polarization profiles revealed a tendency of the alignment between the spin and velocity directions in neutron stars. We study…

astro-ph2006

Black hole mass and accretion rate of Active Galactic Nuclei

Xue-Bing Wu, F. K. Liu, R. Wang +2

The determination of the central black hole mass is crucial to the understanding of AGN physics. In this paper we briefly review some methods that are currently used to estimate th…

astro-ph2006

Arecibo and the ALFA Pulsar Survey

J. van Leeuwen, J. M. Cordes, D. R. Lorimer +34

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.